The resulting sharp observations clearly showed that the closer the stars were to
the very center of the galaxy, the faster they orbited; and the innermost stars were moving as fast as.5 percent the speed of light, or about 900 miles per second.
ALMA's light - gathering capabilities increase the EHT's ability to detect the faint light from
the very center of our galaxy.
Not exact matches
It means that the earth on which we live is not the
center of the physical universe, but a comparatively small planet revolving round a
very average - sized star, which in turn is but one
of a hundred thousand million others forming the
galaxy we call the Milky Way, and that part
of the universe that our existing telescopes have so far penetrated contains about a hundred million star systems or nebulae, similar to our
galaxy.
We see
very strong evidence right at the
center of our own
galaxy.
Previously, astronomers have used x-ray telescopes to observe strong winds
very near the massive black holes at galactic
centers (artist's concept, inset) and infrared wavelengths to detect the vast outflows
of cool gas (bluish haze in artist's concept, main image) from such
galaxies as a whole, but they've never done so in the same
galaxy.
The tendency
of very massive
galaxies to contain a high fraction
of low - mass stars at their
centers is a recent discovery, and is still in some ways controversial, but is reinforced by the work reported here.
New observations from ESO's
Very Large Telescope show for the first time a gas cloud being ripped apart by the supermassive black hole at the
center of the
galaxy.
Using NASA's super-sensitive Chandra X-ray space telescope, a team
of astronomers led by Q. Daniel Wang at the University
of Massachusetts Amherst has solved a long - standing mystery about why most super massive black holes (SMBH) at the
centers of galaxies have such a low accretion rate — that is, they swallow
very little
of the cosmic gases available and instead act as if they are on a severe diet.
The
center of the
galaxy M 82 at
very long radio wavelengths (2.5 m / 118 MHz [orange] and 1.9 m / 154 MHz [blue]-RRB- is depicted.
The sharp Hubble and Keck Observatory images allowed the research teams to separate out the background source star from its neighbors in the
very crowded star field in the direction
of our
galaxy's
center.
Quasars are
very luminous objects powered by accretion
of gas into supermassive black holes at the
centers of distant
galaxies.
«What we observe in this
galaxy is
very much like a massive ocean wave barreling toward shore until it interacts with the shallows, causing it to lose momentum and dump all
of its water and sand on the beach,» said Bruce Elmegreen, a scientist with IBM's T.J. Watson Research
Center in Yorktown Heights, New York, and co-author on the paper.
Kapteyn found that our Sun lies at the
very center of a nearly spherical distribution
of stars, and he incorrectly concluded that we lie at the
center of the
galaxy.
See images
of new observations from ESO's
Very Large Telescope showing a gas cloud ripped apart by the supermassive black hole at the
center of our
galaxy, the Milky Way.
«We expect dark matter to accumulate in the innermost regions
of the Milky Way and other
galaxies, which is why finding such a compact signal is
very exciting,» lead researcher Pierrick Martin, an astrophysicist at the National
Center for Scientific Research and the Research Institute in Astrophysics and Planetology in Toulouse, France, said in a statement.
The research team led by Satoru Iguchi, Associate Professor
of NAOJ, succeeded in observing a
very close binary black hole in the
center of 3C66B (a giant elliptical
galaxy within the cluster A347) just before its black hole merger.
A peek at the
center of our
galaxy, courtesy
of the ESO's
Very Large Telescope, with Sagittarius A *, our galactic black hole, and S2, a daredevil star that orbits relatively close to Sgr A *, highlighted.
The position
of the supermassive black hole at the
center of our Milky Way
galaxy, as well as the giant star S2, are shown (inset) in this near - infrared image from the European Southern Observatory's
Very Large Telescope in Chile.
The halos around quasars — the brightest and the most active objects in the universe, they are
galaxies formed less than 2 billion years after the Big Bang; they have supermassive black holes in their
centers and consume stars, gas, interstellar dust and other material at a
very fast rate — are made
of gas known as the intergalactic medium and extend for up to 300,000 light - years from the
centers of the quasars.
In fact, the bloated core is more than three times larger than the
center of other
very luminous
galaxies.
But we haven't fully connected our theories to what we observe, especially with quasars, these incredibly bright
centers of very distant
galaxies that serve as beacons
of the early universe.
Rufus remains the biggest ass in the
galaxy, his self -
centered quips and firm belief that he's the greatest thing ever making him a
very take him or leave him kind
of hero.